3D Temperature Distribution
High Resolution Picture
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396 KB
(Indeo 5.10)
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ca. 17 MB
(DivX 4)
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4.5 MB
(4.53 MB)
4.53 MB
Temperature dsitributionin a (10 Mpc)^3 cube. The infall of several subclusters onto the cluster centre and the resulting temperature evolution of ICM can be seen. The simulation starts at z=1 and extends to roughly 10 Gyrs into the future.
Institute for Astrophysics, University of Innsbruck